COBRAS/SAMBA - THE ESA MEDIUM-SIZE MISSION FOR MEASUREMENTS OF CBR ANISOTROPY

被引:11
作者
MANDOLESI, N
BERSANELLI, M
CESARSKY, C
DANESE, L
EFSTATHIOU, G
GRIFFIN, M
LAMARRE, JM
NORGAARDNIELSEN, HU
PACE, O
PUGET, JL
RAISANEN, A
SMOOT, GF
TAUBER, J
VOLONTE, S
机构
[1] CNR,IST FIS COSM,I-20133 MILAN,ITALY
[2] CNR,IST TESRE,I-40126 BOLOGNA,ITALY
[3] CENS,CEA,DSM,DAPNIA,SAP,SACLAY,FRANCE
[4] UNIV PADUA,PADUA,ITALY
[5] UNIV OXFORD,OXFORD,ENGLAND
[6] UNIV LONDON QUEEN MARY & WESTFIELD COLL,LONDON E1 4NS,ENGLAND
[7] INST ASTROPHYS SPATIALE,ORSAY,FRANCE
[8] DANISH SPACE RES INST,DK-2800 LYNGBY,DENMARK
[9] ESA,ESTEC,FUTURE PROJECT STUDY OFF,NOORDWIJK,NETHERLANDS
[10] HELSINKI UNIV TECHNOL,SF-02150 ESPOO,FINLAND
[11] UNIV CALIF BERKELEY,LAWRENCE BERKELEY LAB,BERKELEY,CA
[12] ESA,ESTEC,DEPT SPACE SCI,NOORDWIJK,NETHERLANDS
[13] ESA,HQ,DIRECTORATE SCI PROGRAMMES,PARIS,FRANCE
关键词
D O I
10.1016/0032-0633(95)99285-T
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The COBRAS/SAMBA mission is designed for extensive, accurate mapping of the anisotropy of the cosmic Background Radiation, with angular sensitivity from scales of a few arcminutes up to and over-lapping with the > 7 degrees COBE-DMR resolution. This will allow a full identification of the primordial density perturbations which grew to form the large-scale structures observed in the present universe. The COBRAS/SAMBA maps will provide a major source of information relevant to several cosmological and astrophysical issues, such as testing theories of the early universe and the origin of cosmic structure. One of the main diffuse foreground emissions will be from interstellar dust, and the mission will provide relevant information on its components and emission properties. A combination of bolometric and radiometric detection techniques will ensure the sensitivity and wide spectral coverage required for accurate foreground discrimination. A far-Earth orbit has been selected to minimize the unwanted emission from the Earth as a source of contamination. The project is currently undergoing a feasibility study within the European Space Agency M3 programme.
引用
收藏
页码:1459 / 1465
页数:7
相关论文
共 21 条
[1]   MEASURING COSMOLOGICAL PARAMETERS WITH COSMIC MICROWAVE BACKGROUND EXPERIMENTS [J].
BOND, JR ;
CRITTENDEN, R ;
DAVIS, RL ;
EFSTATHIOU, G ;
STEINHARDT, PJ .
PHYSICAL REVIEW LETTERS, 1994, 72 (01) :13-16
[2]   SEPARATION OF FOREGROUND RADIATION FROM COSMIC MICROWAVE BACKGROUND ANISOTROPY USING MULTIFREQUENCY MEASUREMENTS [J].
BRANDT, WN ;
LAWRENCE, CR ;
READHEAD, ACS ;
PAKIANATHAN, JN ;
FIOLA, TM .
ASTROPHYSICAL JOURNAL, 1994, 424 (01) :1-21
[3]   MICROWAVE ANISOTROPIES FROM COSMIC DEFECTS [J].
COULSON, D ;
FERREIRA, P ;
GRAHAM, P ;
TUROK, N .
NATURE, 1994, 368 (6466) :27-31
[4]   IMPRINT OF GRAVITATIONAL-WAVES ON THE COSMIC MICROWAVE BACKGROUND [J].
CRITTENDEN, R ;
BOND, JR ;
DAVIS, RL ;
EFSTATHIOU, G ;
STEINHARDT, PJ .
PHYSICAL REVIEW LETTERS, 1993, 71 (03) :324-327
[5]  
DANESE L, 1995, IN PRESS ASTROPHYS L
[6]   COSMIC MICROWAVE BACKGROUND PROBES MODELS OF INFLATION [J].
DAVIS, RL ;
HODGES, HM ;
SMOOT, GF ;
STEINHARDT, PJ ;
TURNER, MS .
PHYSICAL REVIEW LETTERS, 1992, 69 (13) :1856-1859
[7]   DETECTION OF COSMIC MICROWAVE BACKGROUND ANISOTROPY AT 1-DEGREES.8 - THEORETICAL IMPLICATIONS ON INFLATIONARY MODELS [J].
DEBERNARDIS, P ;
DEGASPERIS, G ;
MASI, S ;
VITTORIO, N .
ASTROPHYSICAL JOURNAL, 1994, 433 (01) :L1-L4
[8]   MEASUREMENTS OF ANISOTROPY IN THE COSMIC MICROWAVE BACKGROUND-RADIATION AT 0-DEGREES.5 ANGULAR SCALES NEAR THE STAR GAMMA-URSAE MINORIS [J].
DEVLIN, MJ ;
CLAPP, AC ;
GUNDERSEN, JO ;
HAGMANN, CA ;
HRISTOV, VV ;
LANGE, AE ;
LIM, MA ;
LUBIN, PM ;
MAUSKOPF, PD ;
MEINHOLD, PR ;
RICHARDS, PL ;
SMOOT, GF ;
TANAKA, ST ;
TIMBIE, PT ;
WUENSCHE, CA .
ASTROPHYSICAL JOURNAL, 1994, 430 (01) :L1-L4
[9]   ANISOTROPY IN THE MICROWAVE SKY AT INTERMEDIATE ANGULAR SCALES [J].
DRAGOVAN, M ;
RUHL, JE ;
NOVAK, G ;
PLATT, SR ;
CRONE, B ;
PERNIC, R ;
PETERSON, JB .
ASTROPHYSICAL JOURNAL, 1994, 427 (02) :L67-L70
[10]  
FARQUHAR RW, 1990, OBSERVATORIES EARTH, P391